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Magnetized Particle Motion in γ-Spacetime in a Magnetic Field

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TLDR
In this paper, the authors explored the dynamics of magnetized particles around the compact object in γ-spacetime in the presence of an external asymptotically-uniform magnetic field.
Abstract
In the present work we explored the dynamics of magnetized particles around the compact object in γ-spacetime in the presence of an external asymptotically-uniform magnetic field. The analysis of the circular orbits of magnetized particles around the compact object in the spacetime of a γ-object immersed in the external magnetic field has shown that the area of stable circular orbits of magnetized particles increases with the increase of γ-parameter. We have also investigated the acceleration of the magnetized particles near the γ-object and shown that the center-of-mass energy of colliding magnetized particles increases with the increase of γ-parameter. Finally, we have applied the obtained results to the astrophysical scenario and shown that the values of γ-parameter in the range of γ∈(0.5,1) can mimic the spin of Kerr black hole up to a≃0.85, while the magnetic interaction can mimic the γ-parameter at γ∈(0.8,1) and spin of a Kerr black hole up to a≃0.3.

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Journal ArticleDOI

Test particles dynamics around deformed Reissner-Nordström black hole

TL;DR: In this article, the authors studied the dynamics of neutral, electrically charged and magnetized particles around deformed electrically and magnetically charged Reissner-Nordstr\"om black holes.

Motion and high energy collision of magnetized particles around a Hořava-Lifshitz black hole

TL;DR: In this article, the authors studied the orbits of magnetized particles around Hořava-Lifshitz black hole with mass M$M$ immersed in an asymptotically uniform magnetic field in the infrared approximation when ωM2≫1$\omega M^{2}\gg 1$.
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Particle acceleration around rotating Einstein-Born-Infeld black hole and plasma effect on gravitational lensing

TL;DR: In this paper, the effect of a two-particle collision near the horizon of a rotating EBI black hole on the horizon and the ergosphere structure is investigated, and the effective potential that governs the particle's motion in the spacetime and the innermost stable circular orbits (ISCO) is also studied.
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Dynamics and epicyclic motions of particles around the Schwarzschild–de Sitter black hole in perfect fluid dark matter

TL;DR: In this article, the authors investigated circular orbits for test particles around the Schwarzschild-de Sitter (dS) black hole surrounded by perfect fluid dark matter and determined the region of circular orbits bounded by innermost and outermost stable circular orbits.
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Distinguishing magnetically and electrically charged Reissner–Nordström black holes by magnetized particle motion

TL;DR: In this article, the effects of electric and magnetic charges of the Reissner-Nordstrom (RN) black hole and spin of the rotating Kerr black hole through the dynamics of the magnetized particles were investigated.
References
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Book

The Mathematical Theory of Black Holes

TL;DR: In a course of lectures on the underlying mathematical structures of classical gravitation theory given in 1978, Brandon Carter as discussed by the authors began with the statement ‘If I had been asked five years ago to prepare a course for recent developments in classical gravity theory, I would not have hesitated on the classical theory of black holes as a central topic of discussion. But I am grateful to them for their courtesy in assigning to me this privilege.
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Is the Gravitational-Wave Ringdown a Probe of the Event Horizon?

TL;DR: It is pointed out that this assumption that very compact objects with a light ring will display a similar ringdown stage, even when their quasinormal-mode spectrum is completely different from that of a black hole, is wrong.
Journal ArticleDOI

Black hole in a uniform magnetic field

TL;DR: In this paper, the authors derived the solution for the electromagnetic field occurring when a stationary, axisymmetric black hole is placed in an originally uniform magnetic field aligned along the symmetry axis of the black hole.
Journal ArticleDOI

Gravitational vacuum condensate stars

TL;DR: A new final state of gravitational collapse is proposed, which has no singularities, no event horizons, and a global time and is thermodynamically stable and has no information paradox.
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